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Observing the WHIM with Athena
2016
Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray
We present simulations of the detection probability for absorption lines from ions in the warm and hot ionized medium (WHIM) with Athena in the spectra of Gamma-ray burst afterglows. The simulations are based on Swift XRT lightcurves of these afterglows and are performed using the end-to-end simulation framework SIXTE. We simulate both the case of single and multiple absorption lines, as well as results for line searches in absorption structures from a more complex medium. We show that the
doi:10.1117/12.2234442
fatcat:7xgl4kw365cqxnvsvwzbkddst4